Chirp mass–distance distributions of the sources of gravitational waves

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Table 3.

Thresholds of distinguishability with p-value α = 0.01.

–	GC	S	V1	V2	V3	V5	V6	V7	V8	V9	V10	V11	V12	V13	V14	V15
GC	–	13	8	13	28	10	13	13	10	13	13	10	13	17	13	10
S	17	–	58	155	74	n	n	n	74	n	683	17	155	17	199	121
V1	13	95	–	199	28	95	74	74	22	74	95	13	95	10	95	58
V2	22	121	58	–	95	155	155	95	28	121	199	13	95	13	1832	58
V3	28	35	17	35	–	35	35	45	22	45	35	10	28	45	74	22
V5	17	417	58	155	95	–	n	n	58	n	417	17	95	17	199	121
V6	17	417	58	121	74	n	–	n	58	n	417	17	95	17	199	95
V7	13	417	45	95	74	874	874	–	95	n	199	17	74	17	155	74
V8	8	28	10	13	28	28	35	28	–	35	22	13	17	13	17	17
V9	13	255	45	74	74	417	417	533	95	–	199	17	58	17	121	58
V10	17	1832	58	199	74	n	3000	1431	45	1118	–	17	417	17	199	121
V11	13	3	6	5	3	3	3	3	13	3	3	–	5	3	3	5
V12	17	n	58	199	74	n	n	n	58	n	1431	13	–	17	199	155
V13	8	17	6	10	35	13	17	17	35	17	17	8	13	–	17	10
V14	22	74	28	95	533	74	74	74	28	74	74	13	45	22	–	28
V15	17	326	95	74	35	417	326	255	58	255	326	13	199	17	58	–

Notes. Displayed vertically are the tested model. Displayed horizontally are the models assumed to be correct, i.e. used to generate data O_i. Here, n signifies that the particular pair of models is indistinguishable even after 3000 observations.

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